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Ozone vertical distribution on Mars from SPICAN/MEX UV occultations

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Anni Määttänen
Franck Lefèvre
Sabrina Guilbon
  • Function : Author
  • PersonId : 971328
Constantino Listowski
  • Function : Author
  • PersonId : 914296
Franck Montmessin

Abstract

We have achieved a four-year cli- matology of the O3 vertical distribution using SPICAM UV occultations. The climatology con- firms the overall behaviour of O3, but reveals some discrepancies in comparison with a global climate model. We are presenting here a simple way to overcome the problem when comparing models and observations; direct comparison of slant profiles (i.e., without doing the vertical inversion).
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insu-02333762 , version 1 (25-10-2019)

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  • HAL Id : insu-02333762 , version 1

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Anni Määttänen, Franck Lefèvre, Sabrina Guilbon, Constantino Listowski, Franck Montmessin. Ozone vertical distribution on Mars from SPICAN/MEX UV occultations. Scientific Workshop: “From Mars Express to ExoMars”, ESAC, Feb 2018, Madrid, Spain. 2 p. ⟨insu-02333762⟩
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